Joint Institute for Nuclear Astrophysics

Results: 24



#Item
1Joint Institute for Nuclear Astrophysics R-matrix Analysis of 16O Reactions Three important reactions to nuclear astrophysics populate the compound nucleus 16O. The 15 N(p,γ)16O and the 15N(p,α0)12C reactions form a br

Joint Institute for Nuclear Astrophysics R-matrix Analysis of 16O Reactions Three important reactions to nuclear astrophysics populate the compound nucleus 16O. The 15 N(p,γ)16O and the 15N(p,α0)12C reactions form a br

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Source URL: www.jinaweb.org

Language: English - Date: 2013-12-11 09:38:47
    2Joint Institute for Nuclear Astrophysics Detection of the Second r-Process Peak Element Tellurium in Metal-Poor Stars Using near-ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on board the Hub

    Joint Institute for Nuclear Astrophysics Detection of the Second r-Process Peak Element Tellurium in Metal-Poor Stars Using near-ultraviolet spectra obtained with the Space Telescope Imaging Spectrograph on board the Hub

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    Source URL: www.jinaweb.org

    Language: English - Date: 2013-12-11 09:38:40
      3Joint Institute for Nuclear Astrophysics High-Resolution Spectroscopic Observations of a Large Sample of VMP Stars from SDSS/SEGUE JINA researchers and colleagues have recently determined chemical compositions, based on

      Joint Institute for Nuclear Astrophysics High-Resolution Spectroscopic Observations of a Large Sample of VMP Stars from SDSS/SEGUE JINA researchers and colleagues have recently determined chemical compositions, based on

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      Source URL: www.jinaweb.org

      Language: English - Date: 2013-12-11 09:39:25
        4Joint Institute for Nuclear Astrophysics Charged Particle Reaction Predictions for NIF To use NIF for astrophysical studies requires a detailed knowledge of density and temperature environment. Charged particle reactions

        Joint Institute for Nuclear Astrophysics Charged Particle Reaction Predictions for NIF To use NIF for astrophysical studies requires a detailed knowledge of density and temperature environment. Charged particle reactions

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        Source URL: www.jinaweb.org

        Language: English - Date: 2013-12-11 09:39:28
          5Joint Institute for Nuclear Astrophysics HST Abundances of Heavy Elements in the U-rich EMP Star CSThe origin and site(s) of the r-process nucleosynthesis is(are) still not known with certainty, but complete,

          Joint Institute for Nuclear Astrophysics HST Abundances of Heavy Elements in the U-rich EMP Star CSThe origin and site(s) of the r-process nucleosynthesis is(are) still not known with certainty, but complete,

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          Source URL: www.jinaweb.org

          Language: English - Date: 2013-12-11 09:39:26
            6Joint Institute for Nuclear Astrophysics Very Metal-Poor Halo Stars with Round Orbits The orbital motions of halo stars in the Milky Way reflect the orbital motions of the progenitor systems in which they formed, making

            Joint Institute for Nuclear Astrophysics Very Metal-Poor Halo Stars with Round Orbits The orbital motions of halo stars in the Milky Way reflect the orbital motions of the progenitor systems in which they formed, making

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            Source URL: www.jinaweb.org

            Language: English - Date: 2013-12-11 09:39:26
              7Joint Institute for Nuclear Astrophysics The First “Fair” Metallicity Distribution Function of the Galactic Halo from SDSS [Fe/H]phot

              Joint Institute for Nuclear Astrophysics The First “Fair” Metallicity Distribution Function of the Galactic Halo from SDSS [Fe/H]phot

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              Source URL: www.jinaweb.org

              Language: English - Date: 2013-12-11 09:39:25
                8Joint Institute for Nuclear Astrophysics Initial Tests for the New 5MV Accelerator A major equipment upgrade at the University of Notre Dame’s Nuclear Science Laboratory, has recently seen the installation of the new S

                Joint Institute for Nuclear Astrophysics Initial Tests for the New 5MV Accelerator A major equipment upgrade at the University of Notre Dame’s Nuclear Science Laboratory, has recently seen the installation of the new S

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                Source URL: www.jinaweb.org

                Language: English - Date: 2013-12-11 09:39:31
                  9Joint Institute for Nuclear Astrophysics Statistical Chemical Tagging in the Smooth Halo Schlaufman et alhave shown that the relative contribution of satellite galaxies accreted at high redshift to the stellar p

                  Joint Institute for Nuclear Astrophysics Statistical Chemical Tagging in the Smooth Halo Schlaufman et alhave shown that the relative contribution of satellite galaxies accreted at high redshift to the stellar p

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                  Source URL: www.jinaweb.org

                  Language: English - Date: 2013-12-11 09:38:40
                    10Joint Institute for Nuclear Astrophysics 22Ne(α,n)26Mg, Neutron source for the weak s-process: exploring the α-threshold in 26Mg Core He- burning in massive stars is the main site for the nucleosynthesis of the light s

                    Joint Institute for Nuclear Astrophysics 22Ne(α,n)26Mg, Neutron source for the weak s-process: exploring the α-threshold in 26Mg Core He- burning in massive stars is the main site for the nucleosynthesis of the light s

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                    Source URL: www.jinaweb.org

                    Language: English - Date: 2013-12-11 09:39:32